[en] We select a close 'major-merger candidate' galaxy pair sample in order to calculate the K_s luminosity function (LF) and pair fraction representative of the merger/interaction component of galaxy evolution in the local universe. The pair sample (projected separation 5 h ^-1 kpc ≤ r≤ 20 h ^-1 kpc, K_s -band magnitude difference ΔK_s ≤ 1 mag) is selected by combining the Two Micron All Sky Survey (2MASS) with the Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5). The resulting data set contains 340 galaxies covering 5800 deg². A stellar mass function is also translated from the LF. A differential pair fraction displays nearly constant fraction of galaxy pairs as a function of galaxy mass from 10⁹ to 10^11.5 M _sun. The differential pair fraction is less subject to absolute magnitude bias due to survey limitations than the standard total pair fraction. These results suggest that major-merger candidate pairs in the 0< z<0.1 universe are developed from ∼1.6% of the galaxy population without dependence on galaxy mass for pair components below 10¹¹ M _sun. The derived LF combined with merger model timescales give local merger rates per unit volume which decrease with masses greater than 10¹¹ M _sun.